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🇺🇦 #NowPlaying on BBCRadio3's #Breakfast
Jean Sibelius, Gothenburg Symphony Orchestra & Santtu-Matias Rouvali:
🎵 Symphony No 2 in D major, Op 43 (1st mvt)
#JeanSibelius #GothenburgSymphonyOrchestra #SanttuMatiasRouvali
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Quantum-Ready Microwave Detection with Scalable Graphene Bolometers in the Strong Localization Regime
Yu-Cheng Chang (Pico group, QTF Centre of Excellence, Department of Applied Physics, Aalto University, Finland), Federico Chianese (Department of Microtechnology and Nanoscience, Chalmers University of Technology, Gothenburg, Sweden), Naveen Shetty (Department of Microtechnology and Nanoscience, Chalmers University of Technology, Gothenburg, Sweden), Johanna Huhtasaari (Department of M…

Quantum-Ready Microwave Detection with Scalable Graphene Bolometers in the Strong Localization Regime
Exploiting quantum interference of charge carriers, epitaxial graphene grown on silicon carbide emerges as a game-changing platform for ultra-sensitive bolometric sensing, featuring an intrinsic resistive thermometer response unmatched by any other graphene variant. By achieving low and uniform carrier densities, we have accessed a new regime of strong charge localization that dramatically reduces thermal conductance, significantly enhancing bolometer performance. Here we present scalable graph…

🇺🇦 #NowPlaying on BBCRadio3's #ThroughTheNight
Franz Berwald, Greta Erikson, Gothenburg Symphony Orchestra & Sten Frykberg:
🎵 Piano Concerto in D major
#FranzBerwald #GretaErikson #GothenburgSymphonyOrchestra #StenFrykberg

Interstellar Polarization Survey. V. Galactic magnetic field tomography in the spiral arms using optical and near-infrared starlight polarization
Y. Angarita (Department of Astrophysics/IMAPP, Radboud University, Nijmegen, The Netherlands, Department of Space, Earth & Environment, Chalmers University of Technology, 412 93 Gothenburg, Sweden), M. J. F. Versteeg (Department of Astrophysics/IMAPP, Radboud University, Nijmegen, The Netherlands), M. Haverkorn (Department of Astrophysics…

Interstellar Polarization Survey. V. Galactic magnetic field tomography in the spiral arms using optical and near-infrared starlight polarization
Interstellar linear polarization occurs when starlight passes through elongated dust grains aligned by interstellar magnetic fields. The observed polarization can come from different dust structures along the line of sight (LOS). By combining polarization measurements with stellar distances, we can study the plane-of-sky Galactic magnetic field (GMF) between the observer and the star and separate the contributions of clouds with different GMF properties. We used optical and near-infrared (NIR) …

🇺🇦 #NowPlaying on BBCRadio3's #EssentialClassics
Jean Sibelius, Gothenburg Symphony Orchestra & Santtu-Matias Rouvali:
🎵 The Wood Nymph, Op 15
#JeanSibelius #GothenburgSymphonyOrchestra #SanttuMatiasRouvali